The two-stage model of protoplanetary matter irradiation

Details The two-stage model of protoplanetary matter irradiation The two-stage model of protoplanetary matter irradiation

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997lpi....28..787l&link_type=abstract

Conference Paper, 28th Annual Lunar and Planetary Science Conference, p. 787.

Astronomy and Astrophysics

Astrophysics

Protoplanets, Irradiation, Rare Gases, Chondrule, Solar Wind, Solar Flares, Meteorites, Magnetic Field Reconnection

Scientific paper

A novel two-stage model of protoplanetary matter irradiation is presently derived from the systematization of (1) data on the content of planetary type and solar type noble gases, as well as (2) precompaction records of the irradiation of constituent grains and chondrules by solar wind and solar flare particles in both gas-rich meteorites and C and O chondrites. Maximum irradiation could have occurred during catastrophic fragmentation and reassembly of parent asteroids.

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